IAS/PU Joint Astrophysics Colloquium

The first light of a core-collapse supernova emerges the moment a shock front breaches the stellar photosphere — just after the star has been engulfed by its explosion, and just before it releases its fastest ejecta. Shock emergence is implicated in...

Turbulence in Planet Formation

Phil Armitage

A combination of sub-mm observations and numerical simulations have the potential to yield direct constraints on the environment of planet formation. After a review of recent observational surprises, I will discuss the implications of our first...

After a basic introduction on how asteroseismology works in practice, we illustrate its application to various kinds of stars of different mass and evolutionary stage. We show how detected oscillation modes allow us to understand details of the...